12.07.2015 Views

Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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Three-dimensional spin foam <strong>Quantum</strong> <strong>Gravity</strong> 307The Lorentzian version of the Ponzano–Regge model is expressed in terms ofthe {6 j} symbols of the non-compact group SO(2, 1) [26]. Holonomies aroundparticles are SO(2, 1) group elements parametrized asg = P 4 + iκ P i τ i with P 2 4 + κ2 P i P i = 1, and P 4 ≥ 0, (16.55)with the metric (+ −−) and the su(1, 1) Pauli matrices, τ 0 = σ 0 ,τ 1,2 = iσ 1,2 .Massive particles correspond <strong>to</strong> the P i P i > 0 sec<strong>to</strong>r. They are described by ellipticgroup elements, P 4 = cos θ, κ|P| =sin θ. The deficit angle is given by the mass,θ = κm. All the mathematical relations of the Riemannian theory are translated <strong>to</strong>the Lorentzian framework by performing the transformationP 0 → P 0 , P 1 → iP 1 , P 2 → iP 2 . (16.56)Note that this transformation differs from a usual Wick rotation (which rotatesP 0 only).The propaga<strong>to</strong>r remains given by the formula (16.41). The momentum spaceis now AdS 3 ∼ SO(2, 1). The addition of momenta is deformed accordingly<strong>to</strong> the formula (16.31). We similarly introduce a group Fourier transform F :C(SO(2, 1)) → C κ (R 3 ) and a ⋆-product dual <strong>to</strong> the convolution product onSO(2, 1). Finally we derive the effective non-commutative field theory with thesame expression (16.43) as in the Riemannian case.It is also possible, in the context of Euclidean gravity, <strong>to</strong> take in<strong>to</strong> account anon-zero cosmological constant . The corresponding model is the Turaev–Viromodel [29] based on U q (SU(2)), where q is on the unit circle for a positive cosmologicalconstant and q is real for a negative cosmological constant. For a positivecosmological constant, provides a maximal length scale. We wrote the explicitFeynman rules corresponding <strong>to</strong> this spin foam model in [4] and showed thatwe obtain a spherical or hyperboloid state sum based on the propaga<strong>to</strong>rs on the3-sphere or the 3-hyperboloid respectively depending on the sign of . Furtherwork is needed <strong>to</strong> analyze the details of these models and extend the results <strong>to</strong> theLorentzian case.To sum up, we have shown how the Ponzano–Regge spin foam model canbe properly gauge fixed in order <strong>to</strong> provide a proper definition of 3d euclidean<strong>Quantum</strong> <strong>Gravity</strong>. We have seen how this model can be naturally coupled <strong>to</strong> matterand that the corresponding 3d <strong>Quantum</strong> <strong>Gravity</strong> amplitudes are actually theFeynman diagram evaluations of a braided and non-commutative QFT. This effectivefield theory describes the dynamics of the matter field after integration of thegravitational degrees of freedom. The theory is invariant under a κ-deformation ofthe Poincaré algebra, which acts non-trivially on many-particle states. This is anexplicit realization of a QFT in the framework of deformed special relativity (seee.g. [30]), which implements from first principles the original idea of Snyder [31]of using a curved momentum space <strong>to</strong> regularize the Feynman diagrams.

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